arxiv.org/abs/2606.30594 Efficient Eccentric Effective-One-Body Dynamics via Near-Identity Averaging Transformations
Researchers present a way to speed up eccentric effective-one-body models of black hole binary inspirals by averaging away fast orbital oscillations. Inspiral dynamics cost drops by up to two orders of magnitude, overall waveform generation is 1.5-8 times faster, and mismatches stay at or below 8.05e-5.
— via arXiv — Astro-ph, Philip Lynch, Alessandra Buonanno, Aldo Gamboa, Maarten van de Meent